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Anharmonic Oscillator by Perturbation Theory

This worked example computes the leading perturbative corrections for the quartic anharmonic oscillator

H=P22m+12mω2X2+λX4,λ>0.H = \frac{P^2}{2m} + \frac12m\omega^2X^2 + \lambda X^4, \qquad \lambda\gt0.

In this worked problem, ΔEn(r)\Delta E_n^{(r)} denotes the physical order-rr contribution and therefore includes the corresponding power of λ\lambda.

The unperturbed problem is the harmonic oscillator, and the perturbation is

V=λX4.V=\lambda X^4.

Use nondegenerate time-independent perturbation theory because the one-dimensional harmonic oscillator has isolated energy levels

En(0)=ℏω(n+12).E_n^{(0)} = \hbar\omega \left(n+\frac12\right).

The small parameter is the size of the quartic energy in the oscillator ground-state width compared with ℏω\hbar\omega:

g=λℏm2ω3.g = \frac{\lambda\hbar}{m^2\omega^3}.

Low-order perturbation theory is plausible when g≪1g\ll1 and the state number nn is not so large that the quartic term dominates.

Write

X=xzpf(a+a†),xzpf=ℏ2mω.X = x_{\mathrm{zpf}} \left(a+a^\dagger\right), \qquad x_{\mathrm{zpf}} = \sqrt{\frac{\hbar}{2m\omega}}.

Then

X4=xzpf4(a+a†)4.X^4 = x_{\mathrm{zpf}}^4 \left(a+a^\dagger\right)^4.

The diagonal matrix element is

⟨n∣X4∣n⟩=xzpf4(6n2+6n+3).\langle n|X^4|n\rangle = x_{\mathrm{zpf}}^4 \left( 6n^2+6n+3 \right).

This can be found by normal ordering, by repeated action of a+a†a+a^\dagger, or by using known oscillator moments.

The first-order correction is

ΔEn(1)=λ⟨n∣X4∣n⟩.\Delta E_n^{(1)} = \lambda\langle n|X^4|n\rangle.

Therefore

ΔEn(1)=λ(ℏ2mω)2(6n2+6n+3).\Delta E_n^{(1)} = \lambda \left( \frac{\hbar}{2m\omega} \right)^2 \left( 6n^2+6n+3 \right).

Equivalently,

ΔEn(1)=λ3ℏ24m2ω2(2n2+2n+1).\Delta E_n^{(1)} = \lambda \frac{3\hbar^2}{4m^2\omega^2} \left( 2n^2+2n+1 \right).

For the ground state,

ΔE0(1)=3λℏ24m2ω2.\Delta E_0^{(1)} = \frac{3\lambda\hbar^2}{4m^2\omega^2}.

For the ground state,

ΔE0(2)=∑r≠0∣⟨r∣λX4∣0⟩∣2E0(0)−Er(0).\Delta E_0^{(2)} = \sum_{r\ne0} \frac{ |\langle r|\lambda X^4|0\rangle|^2 }{ E_0^{(0)}-E_r^{(0)} }.

Parity implies that only even rr can contribute. Repeated ladder-operator action gives

X4∣0⟩=xzpf4(3∣0⟩+62 ∣2⟩+26 ∣4⟩).X^4\lvert0\rangle = x_{\mathrm{zpf}}^4 \left( 3\lvert0\rangle + 6\sqrt2\,\lvert2\rangle + 2\sqrt6\,\lvert4\rangle \right).

Thus only ∣2⟩\lvert2\rangle and ∣4⟩\lvert4\rangle contribute to the sum:

ΔE0(2)=λ2xzpf8[∣62∣2E0(0)−E2(0)+∣26∣2E0(0)−E4(0)]=λ2xzpf8[72−2ℏω+24−4ℏω].\begin{aligned} \Delta E_0^{(2)} =& \lambda^2x_{\mathrm{zpf}}^8 \left[ \frac{|6\sqrt2|^2}{E_0^{(0)}-E_2^{(0)}} + \frac{|2\sqrt6|^2}{E_0^{(0)}-E_4^{(0)}} \right] \\ =& \lambda^2x_{\mathrm{zpf}}^8 \left[ \frac{72}{-2\hbar\omega} + \frac{24}{-4\hbar\omega} \right]. \end{aligned}

Therefore

ΔE0(2)=−42λ2xzpf8ℏω=−21λ2ℏ38m4ω5.\Delta E_0^{(2)} = - \frac{42\lambda^2x_{\mathrm{zpf}}^8}{\hbar\omega} = - \frac{21\lambda^2\hbar^3}{8m^4\omega^5}.

The ground-state energy through second order is

E0=12ℏω+3λℏ24m2ω2−21λ2ℏ38m4ω5+O(λ3).E_0 = \frac12\hbar\omega + \frac{3\lambda\hbar^2}{4m^2\omega^2} - \frac{21\lambda^2\hbar^3}{8m^4\omega^5} + O(\lambda^3).

In terms of

g=λℏm2ω3,g=\frac{\lambda\hbar}{m^2\omega^3},

this is

E0ℏω=12+34g−218g2+O(g3).\frac{E_0}{\hbar\omega} = \frac12 + \frac34g - \frac{21}{8}g^2 + O(g^3).

The first correction is small compared with the unperturbed ground energy when

g≪1.g\ll1.

The second-order term is smaller than the first when, roughly,

21g2/83g/4=72g≪1.\frac{21g^2/8}{3g/4} = \frac72g \ll1.

This numerical estimate is not a rigorous bound, but it is a useful warning: even for the ground state, the second-order coefficient is sizable.

For high nn, the first-order shift grows like n2n^2, while the unperturbed energy grows like nn. A perturbative treatment valid for low states can fail for highly excited states.

The correction has the right dimensions: λX4\lambda X^4 is an energy.

The first-order shift is positive for λ>0\lambda\gt0, as expected for a positive added potential. The second-order shift is negative because excited-state denominators satisfy

E0(0)−Er(0)<0.E_0^{(0)}-E_r^{(0)}\lt0.

Parity is respected: X4X^4 connects the ground state only to even oscillator states.

  • Forgetting that the perturbation is λX4\lambda X^4, not just X4X^4.
  • Dropping off-diagonal matrix elements when computing second order.
  • Missing the ∣4⟩\lvert4\rangle contribution in X4∣0⟩X^4\lvert0\rangle.
  • Assuming a positive perturbing potential gives positive corrections at every perturbative order.
  • Treating the asymptotic perturbation series as a convergent power series.
  • C. M. Bender and T. T. Wu, “Anharmonic oscillator,” Physical Review 184, 1231-1260, 1969.
  • C. M. Bender and T. T. Wu, “Anharmonic oscillator. II. A study of perturbation theory in large order,” Physical Review D 7, 1620-1636, 1973.
  • R. Shankar, Principles of Quantum Mechanics, 2nd ed., Springer, 1994.
  • J. J. Sakurai and J. Napolitano, Modern Quantum Mechanics, 3rd ed., Cambridge University Press, 2020.
  1. Show that
⟨1∣X4∣1⟩=15xzpf4.\langle1|X^4|1\rangle = 15x_{\mathrm{zpf}}^4.
Solution

Use the diagonal formula

⟨n∣X4∣n⟩=xzpf4(6n2+6n+3).\langle n|X^4|n\rangle = x_{\mathrm{zpf}}^4(6n^2+6n+3).

For n=1n=1,

6+6+3=15.6+6+3=15.
  1. Why does a cubic perturbation λX3\lambda X^3 give no first-order energy shift for oscillator eigenstates?
Solution

Harmonic oscillator eigenstates have definite parity. The operator X3X^3 is odd under parity, so

⟨n∣X3∣n⟩=0.\langle n|X^3|n\rangle=0.

The leading nonzero energy shift from a cubic perturbation therefore occurs at second order, assuming the perturbative setup is physically meaningful.